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In this paper we discuss an application of machine learning based methods to the identification of candidate AGN from optical survey data and to the automatic classification of AGNs in broad classes. We applied four different machine…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-14 Stefano Cavuoti , Massimo Brescia , Raffaele D'Abrusco , Giuseppe Longo , Maurizio Paolillo

The latest source catalog of the Fermi-LAT telescope contains more than 7000 $\gamma$-ray sources at GeV energies, with the two dominant source classes thought to be blazars and rotation-powered pulsars. Our target is the identification of…

High Energy Astrophysical Phenomena · Physics 2024-02-09 Martin G. F. Mayer , Werner Becker

We report on the results of deep X-ray follow-up observations of four unidentified Fermi/LAT gamma-ray sources at high Galactic latitudes using Suzaku. The studied objects were detected with high significance during the first 3 months of…

Analysis is presented on 15 months of data taken with the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope for 11 non-blazar AGNs, including 7 FRI radio galaxies and 4 FRII radio sources consisting of 2 FRII radio galaxies…

High Energy Astrophysical Phenomena · Physics 2017-02-22 LAT Collaboration

We reconstruct the extra-galactic gamma-ray source-count distribution, or $dN/dS$, of resolved and unresolved sources by adopting machine learning techniques. Specifically, we train a convolutional neural network on synthetic 2-dimensional…

Cosmology and Nongalactic Astrophysics · Physics 2024-05-16 Aurelio Amerio , Alessandro Cuoco , Nicolao Fornengo

Excess of gamma rays with a spherical morphology around the Galactic center (GC) observed in the Fermi large area telescope (LAT) data is one of the most intriguing features in the gamma-ray sky. The excess has been interpreted by…

High Energy Astrophysical Phenomena · Physics 2024-06-07 Dmitry V. Malyshev

The third catalog of active galactic nuclei (AGNs) detected by the Fermi-LAT (3LAC) is presented. It is based on the third Fermi-LAT catalog (3FGL) of sources detected between 100 MeV and 300 GeV with a Test Statistic (TS) greater than 25,…

High Energy Astrophysical Phenomena · Physics 2015-09-16 M. Ackermann , M. Ajello , W. Atwood , L. Baldini , J. Ballet , G. Barbiellini , D. Bastieri , J. Gonzalez , R. Bellazzini , E. Bissaldi , R. Blandford , E. Bloom , R. Bonino , E. Bottacini , T. Brandt , J. Bregeon , R. Britto , P. Bruel , R. Buehler , S. Buson , G. Caliandro , R. Cameron , M. Caragiulo , P. Caraveo , J. Casandjian , E. Cavazzuti , C. Cecchi , E. Charles , A. Chekhtman , C. Cheung , J. Chiang , G. Chiaro , S. Ciprini , R. Claus , J. Cohen-Tanugi , L. Cominsky , J. Conrad , S. Cutini , R. D'Abrusco , F. D'Ammando , A. Angelis , R. Desiante , S. Digel , L. Venere , P. Drell , C. Favuzzi , S. Fegan , E. Ferrara , J. Finke , W. Focke , A. Franckowiak , L. Fuhrmann , A. Furniss , P. Fusco , F. Gargano , D. Gasparrini , N. Giglietto , P. Giommi , F. Giordano , M. Giroletti , T. Glanzman , G. Godfrey , I. Grenier , J. Grove , S. Guiriec , J. W. Hewitt , A. Hill , D. Horan , G. J'ohannesson , A. Johnson , W. Johnson , J. Kataoka , M. Kuss , G. Mura , S. Larsson , L. Latronico , C. Leto , J. Li , L. Li , F. Longo , F. Loparco , B. Lott , M. Lovellette , P. Lubrano , G. Madejski , M. Mayer , M. Mazziotta , J. McEnery , P. Michelson , T. Mizuno , A. Moiseev , M. Monzani , A. Morselli , I. Moskalenko , S. Murgia , E. Nuss , M. Ohno , T. Ohsugi , R. Ojha , N. Omodei , M. Orienti , E. Orlando , A. Paggi , D. Paneque , J. Perkins , M. Pesce-Rollins , F. Piron , G. Pivato , T. Porter , S. Rain`o , R. Rando , M. Razzano , S. Razzaque , A. Reimer , O. Reimer , R. Romani , D. Salvetti , M. Schaal , F. Schinzel , A. Schulz , C. Sgr`o , E. Siskind , K. Sokolovsky , F. Spada , G. Spandre , P. Spinelli , L. Stawarz , D. Suson , H. Takahashi , T. Takahashi , Y. Tanaka , J. Thayer , J. Thayer , L. Tibaldo , D. Torres , E. Torresi , G. Tosti , E. Troja , Y. Uchiyama , G. Vianello , B. Winer , K. Wood , S. Zimmer

In the forthcoming era of big astronomical data, it is a burden to find out target sources from ground-based and space-based telescopes. Although Machine Learning (ML) methods have been extensively utilized to address this issue, the…

High Energy Astrophysical Phenomena · Physics 2024-01-08 Haitao Cao , Hubing Xiao , Zhijian Luo , Xiangtao Zeng , Junhui Fan

With the advancement of technology, machine learning-based analytical methods have pervaded nearly every discipline in modern studies. Particularly, a number of methods have been employed to estimate the redshift of gamma-ray loud active…

High Energy Astrophysical Phenomena · Physics 2023-12-13 Sarvesh Gharat , Abhimanyu Borthakur , Gopal Bhatta

We present the results of an all-sky radio survey between 5 and 9 GHz of the fields surrounding all unassociated gamma-ray objects listed in the Fermi Large Area Telescope Second Source Catalog (2FGL). The goal of these observations is to…

High Energy Astrophysical Phenomena · Physics 2015-03-12 Frank K. Schinzel , Leonid Petrov , Gregory B. Taylor , Elizabeth K. Mahony , Philip G. Edwards , Yuri Y. Kovalev

Excess of gamma rays around the Galactic center (GC) observed in the Fermi Large Area Telescope (LAT) data is one of the most intriguing features in the gamma-ray sky. The spherical morphology and the spectral energy distribution with a…

High Energy Astrophysical Phenomena · Physics 2025-03-13 Dmitry V. Malyshev

We describe a catalogue of gamma-ray source candidates, selected using the Minimum Spanning Tree (MST) algorithm on the 9-years Fermi-LAT sky (Pass 8) at energies higher than 10 GeV. The extragalactic sky at absolute Galactic latitudes…

High Energy Astrophysical Phenomena · Physics 2018-10-31 R. Campana , E. Massaro , E. Bernieri

We present an updated version catalogue of gamma-ray source candidates, 12Y-MST, selected using the minimum spanning tree (MST) algorithm on the 12-year Fermi-LAT sky (Pass 8) at energies higher than 10 GeV. The high-energy sky at absolute…

High Energy Astrophysical Phenomena · Physics 2021-08-11 R. Campana , E. Massaro

We present the fourth Fermi Large Area Telescope catalog (4FGL) of gamma-ray sources. Based on the first eight years of science data from the Fermi Gamma-ray Space Telescope mission in the energy range from 50 MeV to 1 TeV, it is the…

High Energy Astrophysical Phenomena · Physics 2020-05-27 LAT collaboration

We discuss the time-series behavior of 8 extragalactic 3FGL sources away from the Galactic plane (i.e., $\mid b\mid \geq 10^{\circ}$) whose uncertainty ellipse contains a single X-ray and one radio source. The analysis was done using the…

High Energy Astrophysical Phenomena · Physics 2021-07-14 P. Nkundabakura , J. D. Kamanzi , J. D. Mbarubucyeye , T. Mutabazi

The fourth-DR3 version (4FGL-DR3) of the Fermi/LAT catalogue of $\gamma$-ray sources contains $\sim$ 1000 objects at a galactic latitude |b| > 10$^{\circ}$ which are not identified with an optical counterpart (UGS). We performed a…

High Energy Astrophysical Phenomena · Physics 2024-02-20 Alberto Ulgiati , Simona Paiano , Aldo Treves , Renato Falomo , Boris Sbarufatti , Fabio Pintore , Thomas D. Russell , Giancarlo Cusumano

Fermi-LAT unidentified sources (unIDs) have proven to be compelling targets for performing indirect dark matter (DM) searches. In a previous work, we found that among the 1235 unIDs in Fermi-LAT catalogs (3FGL, 2FHL and 3FHL) only 44 of…

We present an incremental version (4FGL-DR2, for Data Release 2) of the fourth Fermi-LAT catalog of gamma-ray sources. Based on the first ten years of science data in the energy range from 50 MeV to 1 TeV, it uses the same analysis methods…

High Energy Astrophysical Phenomena · Physics 2020-12-18 J. Ballet , T. H. Burnett , S. W. Digel , B. Lott

This is the first of a series of papers aimed at characterizing the populations detected in the high-latitude sky of the {\it Fermi}-LAT survey. In this work we focus on the intrinsic spectral and flux properties of the source sample. We…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-02 LAT Collaboration

Extensive astronomical surveys, like those conducted with the {\em Chandra} X-ray Observatory, detect hundreds of thousands of unidentified cosmic sources. Machine learning (ML) methods offer an efficient, probabilistic approach to classify…

Instrumentation and Methods for Astrophysics · Physics 2026-01-09 Shivam Kumaran , Samir Mandal , Sudip Bhattacharyya
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